Back reaction of Hawking radiation on black hole geometry

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 57, Issue 2, 1998, Pages 1112-1117

  Gegenberg, J ^a  

^a UNIVERSITY OF NEW BRUNSWICK   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0043013916     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.1112     Document Type: Article

References (13)

1. For a discussion and references, see P. Kraus, Ph.D. thesis, Princeton University, 1995.
2. P. Kraus and F. Wilczek, Nucl. Phys. B433, 403 (1995).
3. Nucl. Phys.P. KrausF. WilczekB437, 231 (1995).
4. W. Fischler, D. Morgan, and J. Polchinski, Phys. Rev. D 42, 4042 (1990).
5. M. Henneaux, Phys. Rev. Lett. 54, 959 (1985).
6. J. Gegenberg and G. Kunstatter, Phys. Rev. D 47, R4192 (1993).
7. H. Zaidi and J. Gegenberg, Phys. Lett. B 328, 22 (1994).
8. N. D. Birrel and P. C. W. Davies, Quantum Fields in Curved Space (Cambridge University Press, Cambridge, England, 1982).
9. J. B. Hartle and S. W. Hawking, Phys. Rev. D 13, 2188 (1976).
10. Figures 11a, 11b, 22a and 22b are all MAPLE plots. The units are such that (Formula presented).
11. For a review of the thin shell formalism, see, e.g., M. Visser, Lorentzian Wormholes (AIP Press, New York, 1995), Chap. 14.
12. see also C. Barrabes and W. Israel, Phys. Rev. D 43, 1129 (1991).
13. E. Keski-Vakkuri and P. Kraus, Nucl. Phys. B491, 249 (1997).